activity
20082026
most citedThe Gould's Belt Distances Survey (GOBELINS) I. Trigonometric parallax distances and depth of the Ophiuchus complex

178 citations · 456 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.GA2026

A Radio-Bright Local Little Red Dot Analog

Luis F. Rodriguez, I. FElix Mirabel, Rosa A. Gonzalez-Lopezlira +1

The James Webb Space Telescope revealed the existence in the early Universe ( 4) of large populations of little red dots (LRDs), compact red luminous sources that host rapidly…

astro-ph.GA2020★ 4 cited

On the Thermally Pulsing Asymptotic Giant Branch Contribution to the Light of Nearby Disk Galaxies

Eric E. Martínez-García, Gustavo Bruzual, Rosa A. González-Lópezlira +1

The study of the luminosity contribution from thermally pulsing asymptotic giant branch (TP-AGB) stars to the stellar populations of galaxies is crucial to determine their physical…

astro-ph.GA2018★ 6 cited

Tracers of Stellar Mass-loss - II. Mid-IR Colors and Surface Brightness Fluctuations

Rosa A. González-Lópezlira

I present integrated colors and surface brightness fluctuation magnitudes in the mid-IR, derived from stellar population synthesis models that include the effects of the dusty enve…

astro-ph.GA2017★ 6 cited

The resolved star formation history of M51a through successive Bayesian marginalization

Eric E. Martínez-García, Gustavo Bruzual, Gladis Magris C. +1

We have obtained the time and space-resolved star formation history (SFH) of M51a (NGC 5194) by fitting GALEX, SDSS, and near infrared pixel-by-pixel photometry to a comprehensive…

astro-ph.GA2016★ 20 cited

The relation between globular cluster systems and supermassive black holes in spiral galaxies. The case study of NGC 4258

Rosa A. González-Lópezlira, Luis Lomelí-Núñez, Karla Álamo-Martínez +7

We aim to explore the relationship between globular cluster total number, , and central black hole mass, , in spiral galaxies, and compare it with that recen…

astro-ph.GA2016★ 17 cited

Removing biases in resolved stellar mass-maps of galaxy disks through successive Bayesian marginalization

Eric E. Martínez-García, Rosa A. González-Lópezlira, Gladis Magris C. +1

Stellar masses of galaxies are frequently obtained by fitting stellar population synthesis models to galaxy photometry or spectra. The state of the art method resolves spatial stru…